Minor constituents in the solar wind originating from plasma-dust interactions

Technical Report · Tue Nov 01 00:00:00 EST 1983

OSTI ID:6593571

Ripken, H W

Atoms, molecules, and atomic and molecular ions generated by solar wind interactions with dust grains of the zodiacal cloud are discussed. The main processes leading to the generation of these particles are described and relevant methods of observation are examined.

• Research Organization: Bonn Univ. (Germany, F.R.)
• OSTI ID: 6593571
• Report Number(s): N-84-13116
• Resource Relation: Other Information: In JPL Solar Wind Five, 643-645, see N--84-13067 03-92
• Country of Publication: United States
• Language: English

Related Subjects

71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
SOLAR WIND
MOLECULAR IONS
ATOMS
CARBON
COSMIC DUST
HELIUM
HYDROGEN
INTERACTIONS
IONIZATION
IONS
MASS SPECTROSCOPY
MOLECULES
SILICON
CHARGED PARTICLES
DUSTS
ELEMENTS
FLUIDS
GASES
NONMETALS
RARE GASES
SEMIMETALS
SOLAR ACTIVITY
SPECTROSCOPY
640104* - Astrophysics & Cosmology- Solar Phenomena